telescopecomparison · 2-way
Meade LX200 10" ACF vs Celestron EdgeHD 11
Meade
LX200 10" ACF
Best suited for experienced imagers chasing detail running a permanent observatory setup.
Celestron
EdgeHD 11
Best suited for experienced imagers chasing detail running a permanent observatory setup.
Key differences
-9% focal length
-9% aperture
Specifications
| Specification | Meade LX200 10" ACF | Celestron EdgeHD 11 |
|---|---|---|
| Optics | ||
| Type | sct | sct |
| Optical design | Advanced Coma-Free | Aplanatic SCT |
| Aperture | 254mm | 279mm |
| Focal length | 2540mm | 2800mm |
| Native f/ratio | f/10.0 | f/10.0 |
| Image circle | — | 42mm |
| Full-frame support | No | Yes |
| Physical | ||
| Weight | 13.6kg | 12.7kg |
Advantages of Meade LX200 10" ACF
Closely matched on the compared specs.
Advantages of Celestron EdgeHD 11
- Tighter framing — 2800mm vs 2540mm focal length
- Larger image circle (42mm) — supports bigger sensors
Best for — Meade LX200 10" ACF
- Small galaxies, planetary nebulae, lunar & planetary detail
- High-resolution long-exposure work
- Faint-object imaging under dark skies
Best for — Celestron EdgeHD 11
- Small galaxies, planetary nebulae, lunar & planetary detail
- High-resolution long-exposure work
- Faint-object imaging under dark skies
- Full-frame astro cameras and DSLRs
Meade LX200 10" ACF — typical FOV & scale
- With Full-frame (36×24mm, 3.76µm)FOV: 0.81° × 0.54°Scale: 0.31"/px
- With APS-C (23.5×15.7mm, 3.76µm)FOV: 0.53° × 0.35°Scale: 0.31"/px
- With IMX533 square (11.3×11.3mm, 3.76µm)FOV: 0.25° × 0.25°Scale: 0.31"/px
Celestron EdgeHD 11 — typical FOV & scale
- With Full-frame (36×24mm, 3.76µm)FOV: 0.74° × 0.49°Scale: 0.28"/px
- With APS-C (23.5×15.7mm, 3.76µm)FOV: 0.48° × 0.32°Scale: 0.28"/px
- With IMX533 square (11.3×11.3mm, 3.76µm)FOV: 0.23° × 0.23°Scale: 0.28"/px
Meade LX200 10" ACF — recommended user
Best suited for experienced imagers chasing detail running a permanent observatory setup.
Celestron EdgeHD 11 — recommended user
Best suited for experienced imagers chasing detail running a permanent observatory setup.